Cosmological History: from Gravitational Waves to Exoplanets
Here you can find the slides and the hands-on section exercises we used during the course on Gravitational Wave Astrophysics. Any comment is welcome.
Check school website for further information
Lectures
Lecture 1 Lecture 2 Lecture 3 Lecture 4
Hands-on
Section 1
clone cosmo$\mathcal{R}$ate repository https://gitlab.com/Filippo.santoliquido/cosmo_rate_public
install the conda envirorment following the instruction
activate the envirorment by doing
conda activate cosmo_env
clone
GWFish
git repository at https://github.com/janosch314/GWFishopen and run the notebook
gwfish_tutorial.ipynb
(ignore conda environment instructions)hint :)
Section 2
- download cosmo$\mathcal{R}$ate userguide to learn how to use the code
- Exercises:
- create a figure where you compare the primary mass distribution $m_1$ at different redshifts ($z = 0, 2, 8$) of binary black holes (BBHs) evaluated with two different values of $\sigma_Z = 0.1, 0.6$. Use the astrophysical model provided. Hint: you need to update also the variable
sim_name
- Do the same for BHNSs
- create a figure where you compare the primary mass distribution $m_1$ at different redshifts ($z = 0, 2, 8$) of binary black holes (BBHs) evaluated with two different values of $\sigma_Z = 0.1, 0.6$. Use the astrophysical model provided. Hint: you need to update also the variable
Section 3
- download this Jupyter notebook and this file containing the catalogs (~ 10 MB). Open
jupyter lab
withcosmo_env
kernel in the same folder where you downloaded the data. [A special thank goes to Alessandro Trani for preparing this exercises.]